Abstract
More than 100 evolved, mass losing cool giants have been detected in CO rotational line emission with single-dish telescopes. These observations give information about kinematics, mass loss rates and composition for the evolved stars and can be used to study the evolution to planetary nebulae.
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Knapp, G.R. (1987). Mass Loss from Carbon Stars — Observations of the CO Millimeter Wavelength Rotational Lines. In: Kwok, S., Pottasch, S.R. (eds) Late Stages of Stellar Evolution. Astrophysics and Space Science Library, vol 132. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3813-7_16
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DOI: https://doi.org/10.1007/978-94-009-3813-7_16
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